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202 results on '"Cortese, L."'

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1. WALLABY pilot survey: an ‘almost’ dark cloud near the Hydra cluster

3. PACS photometry of the Herschel Reference Survey – far-infrared/submillimetre colours as tracers of dust properties in nearby galaxies

4. WALLABY pilot survey: an 'almost' dark cloud near the Hydra cluster.

5. The Tully–Fisher relation from SDSS-MaNGA: physical causes of scatter and variation at different radii.

9. WALLABY pilot survey: H i gas disc truncation and star formation of galaxies falling into the Hydra I cluster

10. The SAMI Galaxy Survey: the drivers of gas and stellar metallicity differences in galaxies

11. Deep Extragalactic VIsible Legacy Survey (DEVILS): evolution of the σSFR–M⋆ relation and implications for self-regulated star formation

12. SAMI Galaxy Survey: physical drivers of stellar-gas kinematic misalignments in the nearby Universe.

14. Deep Extragalactic VIsible Legacy Survey (DEVILS): consistent multiwavelength photometry for the DEVILS regions (COSMOS, XMMLSS, and ECDFS)

15. The SAMI Galaxy Survey: the role of disc fading and progenitor bias in kinematic transitions

16. WALLABY pilot survey: first look at the Hydra I cluster and ram pressure stripping of ESO 501−G075

17. physical connection between central stellar surface density and stellar spin in SAMI and MaNGA nearby galaxies.

18. A SAMI and MaNGA view on the stellar kinematics of galaxies on the star-forming main sequence

19. Centrally concentrated molecular gas driving galactic-scale ionized gas outflows in star-forming galaxies

20. WALLABY pilot survey: H i gas disc truncation and star formation of galaxies falling into the Hydra I cluster.

21. SAMI Galaxy Survey: the drivers of gas and stellar metallicity differences in galaxies.

23. From peculiar morphologies to Hubble-type spirals: the relation between galaxy dynamics and morphology in star-forming galaxies at z ∼ 1.5

24. The SAMI Galaxy Survey: first detection of a transition in spin orientation with respect to cosmic filaments in the stellar kinematics of galaxies

25. WALLABY early science − V. ASKAP H i imaging of the Lyon Group of Galaxies 351

27. Galaxy And Mass Assembly (GAMA): Environmental Quenching of Centrals and Satellites in Groups

28. The SAMI Galaxy Survey: observing the environmental quenching of star formation in GAMA groups

29. The SAMI Galaxy Survey: stellar and gas misalignments and the origin of gas in nearby galaxies

31. Galaxy And Mass Assembly (GAMA): The sSFR-M* relation part I – σsSFR-M* as a function of sample, SFR indicator and environment

32. From peculiar morphologies to Hubble-type spirals: the relation between galaxy dynamics and morphology in star-forming galaxies at z ∼ 1.5.

33. The SAMI Galaxy Survey: first detection of a transition in spin orientation with respect to cosmic filaments in the stellar kinematics of galaxies.

34. KROSS–SAMI: a direct IFS comparison of the Tully–Fisher relation across 8 Gyr sincez ≈ 1

35. The SAMI Galaxy Survey: embedded discs and radial trends in outer dynamical support across the Hubble sequence

36. Deep Extragalactic VIsible Legacy Survey (DEVILS): motivation,design, and target catalogue

37. The SAMI Galaxy Survey: gas content and interaction as the drivers of kinematic asymmetry

40. The KMOS Redshift One Spectroscopic Survey (KROSS): the origin of disc turbulence in z ≈ 1 star-forming galaxies

41. Tidal origin of NGC 1427A in the Fornax cluster

42. The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations

43. The SAMI Galaxy Survey: the intrinsic shape of kinematically selected galaxies

44. The SAMI Galaxy Survey: the low-redshift stellar mass Tully–Fisher relation

45. Deriving a multivariate αCO conversion function using the [CII]/CO(1-0) ratio and its application to molecular gas scaling relations

46. The SAMI Galaxy Survey: kinematics of dusty early-type galaxies

47. The SAMI Galaxy Survey: the cluster redshift survey, target selection and cluster properties

49. The SAMI galaxy survey: exploring the gas-phase mass–metallicity relation.

50. SAMI Galaxy Survey: observing the environmental quenching of star formation in GAMA groups.

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